SWIFT J1753.5-0127 was observed by XMM-Newton in March 2006 i.e. after
the end of the first intensive SWIFT campaign covering the outburst
decline. These data are analysed by [1]}, and have much
better signal-to-noise than those of the late decline SWIFT spectra,
but are very similar in shape and intensity. The higher statistics in
these data mean that the soft component is unambiguously
detected, at very high significance. The same spectra model as used in
Table REF  (diskbb+thcomp with absorption fixed at
\(0.2\times 10^{22}\)  cm\(^{-2}\) )gives \(kT_{disc}=0.25\pm 0.01\)  keV and
norm of \(1080\pm 100\) .
